A note on bolometric corrections for late-type stars and long-period variables

Details A note on bolometric corrections for late-type stars and long-period variables A note on bolometric corrections for late-type stars and long-period variables

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..247b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, March 1984, p. 247-249.

Astronomy and Astrophysics

Astronomy

120

Astronomical Photometry, Bolometers, Late Stars, Variable Stars, Correction, Stellar Color

Scientific paper

The results of broad-band BVRcIcJHKL' photometry of late-type stars are used to define a bolometric correction BCIc as a function of (V-I)c or (R-I)c, where mbol = Ic + BCIc. The bolometric corrections BCH and BCK are also derived, and simple analytic expressions are given for BCIc, BCH, and BCK as functions of color index.

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